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Open AccessArticle

Clifford Odd and Even Objects in Even and Odd Dimensional Spaces Describing Internal Spaces of Fermion and Boson Fields

by

Norma Susana Mankoč Borštnik

Symmetry 2023, 15(4), 818; https://doi.org/10.3390/sym15040818 - 28 Mar 2023

Viewed by 619

Abstract

In a long series of works, it has been demonstrated that the spin-charge-family theory, assuming a simple starting action in even dimensional spaces with

d \geq (13 + 1)

, with massless fermions interacting with gravity only, offers the explanation for [...] Read more.

In a long series of works, it has been demonstrated that the spin-charge-family theory, assuming a simple starting action in even dimensional spaces with

d \geq (13 + 1)

, with massless fermions interacting with gravity only, offers the explanation for all assumed properties of the second quantized fermion and boson fields in the standard model, as well as offering predictions and explanations for several of the observed phenomena. The description of the internal spaces of the fermion and boson fields by the Clifford odd and even objects, respectively, justifies the choice of the simple starting action of the spin-charge-family theory. The main topic of the present article is the analysis of the properties of the internal spaces of the fermion and boson fields in odd dimensional spaces,

d = (2 n + 1)

, which can again be described by the Clifford odd and even objects, respectively. It turns out that the properties of fermion and boson fields differ essentially from their properties in even dimensional spaces, resembling the ghosts needed when looking for final solutions with Feynman diagrams. Full article

(This article belongs to the Special Issue Symmetry beyond the Standard Models of Cosmology, High Energy Physics and Quantum Field Theory)

Open AccessArticle

Charge Asymmetry of New Stable Families in Baryon Asymmetrical Universe

by

Vitaly A. Beylin

,

Maxim Yu. Khlopov

and

Danila O. Sopin

Symmetry 2023, 15(3), 657; https://doi.org/10.3390/sym15030657 - 06 Mar 2023

Viewed by 451

Abstract

The new stable fermion family, with Standard Model electroweak (EW) charges, should take part in sphaleron transitions in the early Universe before breaking of the EW symmetry. The conditions of balance between the excess of new fermions (additional generation of new superheavy U, [...] Read more.

The new stable fermion family, with Standard Model electroweak (EW) charges, should take part in sphaleron transitions in the early Universe before breaking of the EW symmetry. The conditions of balance between the excess of new fermions (additional generation of new superheavy U, D quarks and new E, N leptons) and baryon asymmetry, were considered at temperatures above, and below, the phase transition, using a system of equations for chemical potentials. Full article

(This article belongs to the Special Issue Symmetry beyond the Standard Models of Cosmology, High Energy Physics and Quantum Field Theory)

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Open AccessArticle

Gravitational Waves from the Merger of Two Primordial Black Hole Clusters

by

Yury Eroshenko

and

Viktor Stasenko

Symmetry 2023, 15(3), 637; https://doi.org/10.3390/sym15030637 - 03 Mar 2023

Cited by 3 | Viewed by 527

Abstract

The orbital evolution of a binary system consisting of two primordial black hole clusters is investigated. Such clusters are predicted in some theoretical models with broken symmetry in the inflation Lagrangian. A cluster consists of the most massive central black hole surrounded by [...] Read more.

The orbital evolution of a binary system consisting of two primordial black hole clusters is investigated. Such clusters are predicted in some theoretical models with broken symmetry in the inflation Lagrangian. A cluster consists of the most massive central black hole surrounded by many smaller black holes. Similar to single primordial black holes, clusters can form gravitationally bounded pairs and merge during their orbital evolution. The replacement of single black holes by such clusters significantly changes the entire merger process and the final rate of gravitational wave bursts in some parameter ranges (with sufficiently large cluster radii). A new important factor is the tidal gravitational interaction of the clusters. It leads to an additional dissipation of the orbital energy, which is transferred into the internal energy of the clusters or carried away by black holes flying out of the clusters. Comparison with the data of gravitational-wave telescopes allows one to constrain the fractions of primordial black holes in clusters, depending on their mass and compactness. Even the primordial black hole fraction in the composition of dark matter

≃ 1

turns out to be compatible with LIGO/Virgo observational data, if the black holes are in clusters. Full article

(This article belongs to the Special Issue Symmetry beyond the Standard Models of Cosmology, High Energy Physics and Quantum Field Theory)

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Open AccessArticle

Post-Inflationary Production of Dark Matter after Inflection Point Slow Roll Inflation

by

,

,

,

and

Symmetry 2023, 15(2), 543; https://doi.org/10.3390/sym15020543 - 17 Feb 2023

Viewed by 512

Abstract

We explore a feasible model that combines near-inflection point small-field slow roll inflationary scenario driven by single scalar inflaton with the production of non-thermal vector-like fermionic dark matter,

χ

, during the reheating era. For the inflationary scenario, we consider two separate polynomial [...] Read more.

We explore a feasible model that combines near-inflection point small-field slow roll inflationary scenario driven by single scalar inflaton with the production of non-thermal vector-like fermionic dark matter,

χ

, during the reheating era. For the inflationary scenario, we consider two separate polynomial forms of the potential; one is symmetric about the origin, and the other is not. We fix the coefficients of the potentials satisfying current Planck-Bicep data. We calculate the permissible range of

y_{χ}

and

m_{χ}

for the production of enough dark matter to explain the total Cold Dark Matter (CDM) mass density of the present universe while satisfying Cosmic Background Radiation (CMBR) measurements and other cosmological bounds. Full article

(This article belongs to the Special Issue Symmetry beyond the Standard Models of Cosmology, High Energy Physics and Quantum Field Theory)

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Open AccessArticle

Gravitational Baryogenesis: Problems and Possible Resolution

by

,

,

and

Symmetry 2023, 15(2), 404; https://doi.org/10.3390/sym15020404 - 03 Feb 2023

Cited by 1 | Viewed by 394

Abstract

The coupling of baryonic current to the derivative of the curvature scalar, R, inherent to gravitational baryogenesis (GBG), leads to a fourth-order differential equation of motion for R instead of the algebraic one of general relativity (GR). The fourth-order differential equation is [...] Read more.

The coupling of baryonic current to the derivative of the curvature scalar, R, inherent to gravitational baryogenesis (GBG), leads to a fourth-order differential equation of motion for R instead of the algebraic one of general relativity (GR). The fourth-order differential equation is generically unstable. We consider a possible mechanism of stabilization of GBG by the modification of gravity, introducing an

R^{2}

term into the canonical action of GR. It is shown that this mechanism allows for the stabilization of GBG with bosonic and fermionic baryon currents. We establish the region of the model parameters leading to the stabilization of R. Still, the standard cosmology would be noticeably modified. Full article

(This article belongs to the Special Issue Symmetry beyond the Standard Models of Cosmology, High Energy Physics and Quantum Field Theory)

Open AccessArticle

Hot Primordial Regions with Anomalous Hydrogenless Chemical Composition

by

Konstantin M. Belotsky

,

Mohamed M. El Kasmi

,

Sergey G. Rubin

and

Maxim L. Solovyov

Symmetry 2022, 14(7), 1452; https://doi.org/10.3390/sym14071452 - 15 Jul 2022

Viewed by 585

Abstract

We study primordial nucleosynthesis in hypothetical hot regions that could be formed by the primordial density inhomogeneities. It is shown that the regions that survived up to the present times acquire an abnormally high metallicity. This conclusion holds in a wide range of [...] Read more.

We study primordial nucleosynthesis in hypothetical hot regions that could be formed by the primordial density inhomogeneities. It is shown that the regions that survived up to the present times acquire an abnormally high metallicity. This conclusion holds in a wide range of initial parameters of such regions. We considered the thermonuclear reaction rates and estimated abundances of deuterium and helium-3 and -4 inside these areas. It has been established that all baryons tend to form helium-4, which is the thermonuclear link in the chain of formation of heavier elements. Full article

(This article belongs to the Special Issue Symmetry beyond the Standard Models of Cosmology, High Energy Physics and Quantum Field Theory)

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Open AccessArticle

Sub-Planckian Scale and Limits for f(R) Models

by

Polina Petriakova

,

Arkady Popov

and

Sergey Rubin

Symmetry 2021, 13(2), 313; https://doi.org/10.3390/sym13020313 - 13 Feb 2021

Cited by 1 | Viewed by 1111

Abstract

We study the universe evolution starting from the sub-Planckian scale to present times. The requirement for an exponential expansion of the space with the observed metric as a final stage leads to significant restrictions on the parameter values of a function [...] Read more.

We study the universe evolution starting from the sub-Planckian scale to present times. The requirement for an exponential expansion of the space with the observed metric as a final stage leads to significant restrictions on the parameter values of a function

f (R)

. An initial metric of the Universe is supposed to be maximally symmetric with the positive curvature. Full article

(This article belongs to the Special Issue Symmetry beyond the Standard Models of Cosmology, High Energy Physics and Quantum Field Theory)

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Open AccessArticle

Heavy Quark Symmetry and Fine Structure of the Spectrum of Hadronic Dark Matter

by

Vladimir Kuksa

and

Vitaly Beylin

Symmetry 2020, 12(11), 1906; https://doi.org/10.3390/sym12111906 - 20 Nov 2020

Cited by 2 | Viewed by 999

Abstract

We analyze the structure of excited states of new heavy hadrons in the scenario with hadronic dark matter. Fine mass-splitting in a doublet of new mesons stipulates the existence of charged metastable heavy mesons. We describe the structure of new meson excited states [...] Read more.

We analyze the structure of excited states of new heavy hadrons in the scenario with hadronic dark matter. Fine mass-splitting in a doublet of new mesons stipulates the existence of charged metastable heavy mesons. We describe the structure of new meson excited states in the framework of the heavy quark effective theory. Phenomenological consequences of fine and hyperfine splitting are considered in the hadronic dark matter scenario and beyond. Full article

(This article belongs to the Special Issue Symmetry beyond the Standard Models of Cosmology, High Energy Physics and Quantum Field Theory)

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Open AccessConference Report

Copernican Paradigm beyond FLRW

by

Chethan Krishnan

,

Ranjini Mondol

and

M. M. Sheikh Jabbari

Symmetry 2023, 15(2), 428; https://doi.org/10.3390/sym15020428 - 06 Feb 2023

Cited by 1 | Viewed by 397

Abstract

We present the dipole cosmological principle, i.e., the notion that the Universe is a Copernican cosmology that agrees with the cosmic flow. It suits the most symmetric paradigm that generalizes the Friedmann–Lemaître–Robertson–Walker ansatz in the context of numerous suggestions that have appeared in [...] Read more.

We present the dipole cosmological principle, i.e., the notion that the Universe is a Copernican cosmology that agrees with the cosmic flow. It suits the most symmetric paradigm that generalizes the Friedmann–Lemaître–Robertson–Walker ansatz in the context of numerous suggestions that have appeared in the literature for non-kinematic components in the cosmic microwave background dipole. Field equations in our “dipole cosmology” are still ODEs, but we now have four instead of two Friedmann equations. The two extra functions can be regarded as additional scale factors that break the isotropy group from SO(3) to U(1) and a “tilt” that denotes the cosmic flow. The result is an axially isotropic Universe. We examined the dynamics of the expansion rate, anisotropic shear, and tilt in some cases. One important observation is that the cosmic flow (tilt) can grow while the anisotropy (shear) dies down. Full article

(This article belongs to the Special Issue Symmetry beyond the Standard Models of Cosmology, High Energy Physics and Quantum Field Theory)

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